Name | Kepler-62 | ||
Distance | — | ||
Spectral type | K2V | ||
Apparent magnitude V | 14.0 | ||
Mass | 0.69 (± 0.02) MSun | ||
Age | — | ||
Effective temperature | 4869.0 K | ||
Radius | 0.63 (± 0.02) RSun | ||
Metallicity [Fe/H] | -0.21 | ||
Detected Disc | — | ||
Magnetic Field | — | ||
RA2000 | 18:52:51.0 | ||
Dec2000 | +45:20:60 | ||
Alternate Names | |||
Planetary system | 5 planets |
Exo-Milankovitch Cycles I: Orbits and Rotation States
2018
DEITRICK R., BARNES R., QUINN Th., ARMSTRONG J., CHARNEY B. & WILHELM C.
Astron. J., 155, 60
paper arxiv
How alien can alien worlds be?
2017
ADIBEKYAN F., FIGUEIRA P. & SANTOS N.
in EWASS Special Session 4 (2017): Star-planet interactions
arxiv
Orbital Dynamics of Exoplanetary Systems Kepler-62, HD 200964 and Kepler-11
2016
MIA R. & KUSHVAH B.
MNRAS, 457, 1089
paper arxiv
Gravitational quantization of exoplanet orbits in HD 40307, $μ$ Ara, Kepler-26, Kepler-62, and Kepler-275: Comparing predicted orbits
2015
GEROYANNIS V.
arxiv
Mercury-T: A new code to study tidally evolving multi-planet systems. Applications to Kepler-62
2015
BOLMONT E., RAYMOND S., LECONTE J., HERSANT F. & CORREIA A.
Astron. & Astrophys., accepted
arxiv
Habitable Zone Dependence on Stellar Parameter Uncertainties
2014
KANE S.
ApJ, 782, 111
paper arxiv
Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186
2014
BOLMONT E., RAYMOND S., LECONTE J., CORREIA A. & QUINTANA E.
in IAU Symposium No. 310
arxiv
Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone
2013
BORUCKI W., AGOL E., FRESSIN F., KALTENEGGER L., ROWE J. & 59 additional authors
Science, 340, 587
paper arxiv